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Fig. A.3.

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Clockwise starting in the upper left panel: HST F160W image including the galaxy 38910 in the north-east upper part of the image and 38768 in the center, with overplotted [OII] EL map; spatially resolved [OII] EL map; spatially resolved [OII] velocity dispersion map; spatially resolved [OII] velocity map. The white background corresponds to spaxels with S/N[OII] < 3. From ALMA, galaxy 38768 has a derived molecular gas mass of (3.1 ± 0.6)×1010M (Hayashi et al. 2018).

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